On the Shape of Intrinsic Gamma-Ray Spectra of Distant Blazars

Details On the Shape of Intrinsic Gamma-Ray Spectra of Distant Blazars On the Shape of Intrinsic Gamma-Ray Spectra of Distant Blazars

Oct 2010

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2010aspc..427..310z&link_type=abstract

Accretion and Ejection in AGN: a Global View. Proceedings of a conference held June 22-26, 2009 in Como, Italy. Edited by Laura

Physics

Scientific paper

We investigate a way internal absorption can be used to explain the quite hard spectrum observed in some blazars. Starting from the blazar observations in the very high energy (VHE) regime, we continue with deabsorbing these spectra with current Extragalactic Background Light (EBL) models. Then, internal absorption is used to explain the X-ray (through the secondary emission) and γ-ray spectra of two distant blazars, 1ES 0229+200 (z=0.1396) and 3C 66A (z=0.444).

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